8
The assumption we have made here at SBIG is that you will
leave the SG-4 attached to the guide scope and do not change the
focus, or you will mark or scribe or lock down the drawtube so you
can repeat your focus position in the field without a computer, once
you have determined it.
Once you have found the best focus (it is not that critical for
guiding), make sure the phone guiding cable is connected between
your mount and the SG-4. Position an isolated bright 3rd to 5th
magnitude star located within 20 degrees of the celestial equator onto
the center of the SG-4 field using the “Take Image” and
“Continuous” controls, and click “Calibrate Guider”. The guider will
attempt to calibrate the mount speed. A pop-up text window will
appear so you can see the process. The SG-4 starts out with a series
of small moves with the “X” relay, which should be in the Right
Ascension direction, but by no means is necessarily in the X-direction
on the screen or on the CCD. Once it detects movement, it knows the
backlash has been taken out of the mount and it makes a few long
moves to calibrate the speed. Once it finishes in X the SG-4 will
assume the speed in the –X direction is the same, but in the opposite
direction, and it will start the same calibration process in Y. When it
finishes it will display the calibration vectors it found. It is a good
idea to check out these vectors to see if the speeds are reasonable.
Most mounts correct at a speed of around 7.5 arcseconds per second,
which is about 5 pixels per second with a focal length of 1000 mm.
With a 200 mm focal length it will be 1 pixel per second. When the
calibration finishes save your calibration text file so you can send it to
customer service at SBIG if there is a problem. The calibration you
obtain should work at any declination so, as long as you don’t rotate
your camera or the guide scope, or reposition the guide scope on your
main scope, the vectors should be good. If you have a German
Equatorial mount take note of the position of the East/West toggle
switch on the back of the SG-4 and remember to keep it in the same
place when on the same side of the pier. Do not worry about which is
East and which is West – it doesn’t matter as long as you remember
which side of the pier you were on. Note, however, that the SG-4
assumes that +X and –X correspond to RA motion for this switch to
function properly with a GEM. If you flip the telescope to the other
side, flip the switch to flip the calibration vectors. NOTE: if you
forget to flip it the mount will immediately run away in one axis
while tracking, with your corrections getting longer and longer. That
is how you will recognize this problem. Also, if calibration fails, you
will not be able to track.